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International cooperation was once the keynote of the Apollo-Soyuz try out undertaking. within the three y ears because the venture was once initiated within the U.S. - U .S .S .R. contract bearing on Cooperation within the Exploration and Use of Outer area (signed by way of the U.S. and U.S.S .R. Heads of nation on might 24, 1972), the good attempt expended in coordination, conversation, and integration culminated within the hugely profitable flight from July 15 to 24, 1975. The 9-day flight marked the 1st time that manned spacecraft of 2 international locations have met in house for joint engineering and clinical investigations .
The primary goal of the venture was once to strengthen a appropriate docking approach and rendezvous and workforce move methods that will be acceptable for destiny overseas manned area missions. This aim was once effectively complete.
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Additional resources for Apollo-Soyuz Test Project Preliminary Science Report
17, 1972, pp. 155-160. 4-2. Rose, W. ; and Wentzel, D. : Ultraviolet Stars and the Interstellar Gas. Astrophys. , vol. 181, 1973, pp. 115-123. 4-3. Greenstein, J. ; and Sargent, A. : The Nature of Faint Blue Stars in the Halo. II. Astrophys. J. Supp. Series, vol. 28 , no. 259, 1974, pp. 157-210. 4-4. Carnochan, D. ; Dworetsky, M. ; Todd , J. ; Willis, A. : A Search for Ultraviolet Objects. Phil. Trans. Roy . Soc. London, A, vol. 279, 1975, pp. 479 - 485. 4-5. Rogerson, J. ; York, D. ; Drake , J.
Detector Subsystem The detector subsystem was composed of four similar channels, each of which detected photons by means of a channel electron multiplier. Channels 1 and 3 were identical , as were channels 2 and 4. 4-nanometer radiation through helium gas absorption cells. 10 me ter long and was capped with two thin metal filters, one tin and one aluminum. Layers of these elements a few hundred nanometers thick are transparent in the extreme ultraviolet (EUV) spectral region, and the particular combination of fi lters used defines a bandpass approximately 10 nanometers wide, containing the 58.
Figure 4-6. - Positional error box for the EUV source in Coma Berenices derived from the revolution 109 data (solid line). The broken line is the error box for the soft X-ray source observed from Small Astronomy Satellite-3 (ref. 4-15). The white dwarf HZ 43 is also marked in the center of the photograph. Enlargement is from the blue Sky Survey plate (copyright by the National Geographic Society - Palomar Observatory Sky Survey; reproduced by permission of the Hale Observatories). 4- 16 I J 5 .
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